Dynamical evolution of open clusters.

Details Dynamical evolution of open clusters. Dynamical evolution of open clusters.

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988bancc..58..177a&link_type=abstract

Bol. Acad. Nac. Cienc. Cordoba, Argent., Tomo 58, Nos. 3 - 4, p. 177 - 187

Computer Science

Open Clusters: Dynamical Evolution, Open Clusters: Stellar Dynamics, Open Clusters: Numerical Simulations

Scientific paper

The author discusses dynamical models of open star clusters mainly based on the N-body simulations of Terlevich (1983, 1987). A series of self-consistent models with up to 1000 stars of different masses has been studied. Specific effects appropriate to open clusters include the galactic tidal force for a circular orbit, instantaneous loss due to supernova events, and the irregular force of interstellar clouds. The simulations yield information about cluster life-times and the behaviour of different masses, which may be compared with observations.

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